High-Energy Astrophysics — MCQs August 20, 2025 by u930973931_answers 50 Score: 0 Attempted: 0/50 Subscribe 1. What is the primary source of high-energy photons in the universe? (A) Stars (B) Supernovae (C) Black holes and neutron stars (D) Planets 2. X-ray astronomy mainly studies which cosmic objects? (A) Planets (B) Cold molecular clouds (C) Hot and compact objects (D) Globular clusters 3. The Crab Nebula is a strong source of: (A) Radio waves only (B) Gamma rays and X-rays (C) Infrared radiation (D) Optical emission only 4. What is the typical energy range of X-rays? (A) 0.1–10 eV (B) 10–100 eV (C) 0.1–100 keV (D) 1–10 MeV 5. What is the typical energy range of gamma rays? 6. Which type of binary system emits strong X-rays? (A) White dwarf + red giant (B) Neutron star or black hole + companion star (C) Planet + brown dwarf (D) Star + asteroid belt 7. Cygnus X-1 is known as a candidate: (A) Neutron star (B) Quasar (C) Black hole (D) Pulsar 8. What physical process generates synchrotron radiation? (A) Nuclear fusion (B) Acceleration of charged particles in magnetic fields (C) Radioactive decay (D) Dark matter annihilation 9. What is inverse Compton scattering? (A) Photon loses energy to an electron (B) Photon gains energy from an electron (C) Photon absorbed by nucleus (D) Photon splits into two 10. Which space telescope was specifically designed for X-ray astronomy? (A) Hubble (B) Chandra (C) Kepler (D) Spitzer 11. Which space observatory is designed for gamma-ray astronomy? (A) Chandra (B) Fermi (C) Hubble (D) Gaia 12. What is the main power source of gamma-ray bursts (GRBs)? (A) Planet collisions (B) Supernovae or neutron star mergers (C) Cosmic rays hitting dust (D) Quasar jets 13. Short GRBs are generally associated with: (A) Massive star collapse (B) Neutron star mergers (C) Black hole jets (D) Pulsar emissions 14. Long GRBs are usually linked to: (A) Supermassive black holes (B) Supernovae from massive stars (C) White dwarf collapse (D) Galaxy clusters 15. Pulsars are rotating: (A) White dwarfs (B) Neutron stars (C) Black holes (D) Red giants 16. Millisecond pulsars spin with a period of about: (A) Seconds (B) Minutes (C) Hours (D) Milliseconds 17. Magnetars are neutron stars with extremely high: (A) Temperature (B) Magnetic fields (C) Rotation speed (D) Mass 18. Accretion disks around black holes emit strongly in: (A) Infrared (B) Optical (C) X-rays (D) Radio 19. Active Galactic Nuclei (AGN) are strong emitters of: (A) Only optical light (B) Radio, X-ray, and gamma rays (C) Microwave radiation only (D) Infrared only 20. What are jets from AGN mainly composed of? (A) Neutrinos (B) Relativistic particles and plasma (C) Photons only (D) Hydrogen atoms 21. Which galaxy hosts a famous giant radio jet? (A) Andromeda (B) M87 (C) Triangulum (D) Sombrero Galaxy 22. What is the Eddington limit? (A) Maximum temperature of a star (B) Balance between radiation pressure and gravity (C) Maximum speed of jet (D) Limit on black hole mass 23. Pair production occurs when a gamma-ray photon converts into: (A) Proton + neutron (B) Electron + positron (C) Quark + antiquark (D) Neutrino + antineutrino 24. Cosmic rays are primarily composed of: (A) Electrons (B) Protons and atomic nuclei (C) Neutrinos (D) Gamma rays 25. Which experiment studies ultra-high-energy cosmic rays? (A) ALMA (B) Pierre Auger Observatory (C) Chandra (D) Fermi Telescope 26. The “knee” in the cosmic ray spectrum occurs at energies around: (A) 10⁹ eV (B) 10¹⁵ eV (C) 10²⁰ eV (D) 10²³ eV 27. The “ankle” in the cosmic ray spectrum refers to: (A) Low-energy cutoff (B) Transition at ~10¹⁸ eV (C) Maximum energy of pulsars (D) Shock acceleration end 28. The Greisen–Zatsepin–Kuzmin (GZK) cutoff limits cosmic rays above: (A) 10¹⁵ eV (B) 10¹⁸ eV (C) 10²⁰ eV (D) 10²² eV 29. Neutrino astronomy provides information about: (A) Planet formation (B) Extreme astrophysical events (C) Stellar photospheres (D) Interstellar dust 30. The IceCube experiment detects neutrinos using: (A) Space telescopes (B) Antarctic ice Cherenkov radiation (C) Underground detectors only (D) Radio telescopes 31. Supernova 1987A provided the first detection of: (A) Cosmic rays (B) Neutrinos from a stellar explosion (C) X-rays from black holes (D) Gravitational waves 32. Gravitational waves were first detected from: (A) White dwarf collisions (B) Neutron star mergers (C) Black hole mergers (D) Pulsar signals 33. LIGO and Virgo detect gravitational waves using: (A) X-ray telescopes (B) Interferometers (C) Radio antennas (D) Cosmic ray detectors 34. What energy mechanism powers blazars? (A) Nuclear fusion (B) Accretion onto supermassive black holes (C) White dwarf thermonuclear reactions (D) Dark energy 35. The difference between blazars and quasars is due to: (A) Jet orientation (B) Galaxy type (C) Black hole mass (D) Stellar population 36. TeV gamma rays are detected using: (A) Optical telescopes (B) Space X-ray detectors (C) Atmospheric Cherenkov telescopes (D) Infrared cameras 37. Which telescope detects TeV gamma rays? (A) MAGIC (B) Chandra (C) Spitzer (D) Kepler 38. Which telescope is part of a system for ground-based gamma-ray detection? (A) VERITAS (B) Hubble (C) ALMA (D) Gaia 39. The Cherenkov Telescope Array (CTA) is designed for: (A) Neutrino astronomy (B) Gamma-ray astronomy (C) Gravitational wave detection (D) Infrared mapping 40. Which mechanism explains particle acceleration in shocks? (A) Fermi acceleration (B) Nuclear fusion (C) Pair production (D) Inverse decay 41. Relativistic jets emit across which spectrum? (A) Only radio (B) Only X-rays (C) Only optical (D) Across the entire electromagnetic spectrum 42. What limits the speed of jets in AGN? (A) Dark matter drag (B) Relativistic effects and light speed (C) Magnetic confinement (D) Interstellar medium 43. High-energy neutrinos are expected from: (A) Planetary atmospheres (B) AGN jets and GRBs (C) Stellar coronae (D) Globular clusters 44. Which process dominates X-ray binaries? (A) Magnetic reconnection (B) Accretion (C) Stellar winds only (D) Dark energy decay 45. The brightest X-ray binary in the Milky Way is: (A) Cygnus X-1 (B) Hercules X-1 (C) Scorpius X-1 (D) Vela X-1 46. Gamma-ray bursts typically last: (A) Nanoseconds (B) Milliseconds to minutes (C) Years (D) Centuries 47. X-ray pulsars modulate X-rays due to: (A) Orbital motion (B) Rotating magnetic fields (C) Accretion of dark matter (D) Nuclear reactions in crust 48. The high-energy emission of supernova remnants comes from: (A) Thermal dust (B) Accelerated particles (cosmic rays) (C) Planetary systems (D) Stellar winds only 49. Which object emits the most energetic gamma rays in the universe? (A) Stars (B) Pulsars (C) Gamma-ray bursts (D) Supernova remnants 50. High-energy astrophysics helps us probe: (A) Planet formation only (B) Extreme cosmic environments (C) Stellar atmospheres (D) Interstellar dust